The Two Component Magnetic Field of the Galaxy
1990 ◽
Vol 140
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pp. 54-54
Keyword(s):
The present paper is devoted to a study of the magnetic field configuration of our Galaxy based on Faraday rotation measures (RM) of 185 pulsars and 802 extragalactic radio sources. RM data of pulsars located near the plane of the Galaxy are used for the study of magnetic fields in neighbouring spiral arms. For the distribution of spiral arms the well-known model of Georgelin and Georgelin (1976) is used. The calculations show (for details see Andreassian and Makarov, 1987, 1989) that in the Perseus spiral arm and the local Orion arm the magnetic fields have approximately the same directions (lo;bo) ≈ (80°;0°), while in the Sagittarius-Carina arm the magnetic field has an opposite direction.
1998 ◽
Vol 164
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pp. 115-116
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1968 ◽
Vol 35
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pp. 202-210
1970 ◽
Vol 39
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pp. 168-183
Keyword(s):
Keyword(s):
1971 ◽
Vol 43
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pp. 243-248
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1997 ◽
Vol 163
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pp. 799-800
Keyword(s):